RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 5.7980e-04 Jy/beam
minimum 1.1387e-04 Jy/beam
mean 1.8625e-04 Jy/beam
median 1.4718e-04 Jy/beam
sigma 8.3571e-05 Jy/beam
MAD rms 1.3822e-05 Jy/beam

RMS images

VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms

VLASS1.2.ql.T15t26.J185948_193000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t26.J185948+193000_P39036v1_2019_04_02T16_31_54.293/working/VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t26.J185948+193000_P39036v1_2019_04_02T16_31_54.293/working
Start time
2019-04-04 03:22:33.325
End
2019-04-04 03:24:48.708
Duration
0:02:15.382
Note, WebLog generation is not included in the time.

CASA logs for stage 6